Proposal code
w013
Proposal title
Search for the smallest structure in the Galactic molecular clouds
The |
Investigators and their |
Affiliations |
P.I. |
Hiroshi Imai |
Astronomical Institute, Tohoku Univ., Japan |
|
Seiji Kameno |
VSOP project, NAO, Japan |
|
Kazuyoshi Sunada |
Nobeyama Radio Observatory, NAO, Japan |
|
Tetsuo Sasao |
Mizusawa Astrogeodynamics Obs., NAO, Japan |
Proposal Abstract
We propose trial observations to search for the smallest structure in the
Galactic molecular clouds by detecting spatial contrast and its time
variation in the profiles of formaldehyde absorptions towards extragalactic
radio sources. The previous observtions suggest gas structure smaller
than 10 AU, but have never found any lower cutoff of the structure size.
High mapping quality and spatial resolution of VSOP should reveal fine
structure of the background extragalactic sources and their time
variations, and be free ideally from beam dilution to smear the
absorption profiles. We propose to observe suitiable strong sources
near the Galactic plane, 0212+735, DA193, 0528+134, and NRAO530 in
two observing sessions for the each source. Such a study
makes us understand a universal picuture for interstellar molecular clouds
and how density contrast and turbulence, which affect star formation,
are created.
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